Abstract: Telescope time is requested to do astrometry and photometry of carefully selected Near-Earth Objects (NEOs) previously detected by the WISE all-sky thermal infrared (IR) survey. As an infrared survey, WISE was more efficient at finding low albedo solar system objects than ground based surveys, nearly doubling the known population of low albedo NEOs. Albedo-outliers may represent hitherto unexplored populations and may reveal characteristics of the evolution of the solar system not yet recognized. Also, delivery of asteroids from the main belt to Earth- crossing orbits depends on physical properties such as albedo, size, & composition. Measurements of mineralogical classes will refine understanding of the filtering involved in asteroid transport. Astrometry of our targets will refine knowledge of their orbits and ensure later recovery. High signal-to-noise ratio (SNR) R-band photometry on a calibrated magnitude scale establishes the albedo near the peak of incident solar flux, which reckons centrally in modeling thermal properties. BVRI colors allow us to determine approximate taxonomic types.